On the characteristics of 150-km echoes observed in the Brazilian longitude sector by the 30 MHz São Luís radar

dc.contributor.authorRodrigues, F. S.
dc.contributor.authorDe Paula, E. R.
dc.contributor.authorChau Chong Shing, Jorge Luis
dc.date.accessioned2018-07-20T17:02:19Z
dc.date.available2018-07-20T17:02:19Z
dc.date.issued2011-10-28
dc.description.abstractWe present long-overdue details about the intensity and spectral characteristics of 150-km echoes observed by the Sao Lu ıs radar in Brazil. The Sao Lu ıs observations show that the echoes usually come from multiple scattering layers that descend in altitude before local noon, and ascend during afternoon hours, similar to what has been found in observations made in other longitude sectors. The layers are usually 3–5 km thick and located, mostly, between 130 and 170 km altitude. The measurements also show variations in echo intensity that are similar to observations made at other equatorial and off-equatorial sites. Analysis of observations made during 2008 shows significant (>37 %) monthly occurrence rates for every month. Reduced occurrence rates were observed around March Equinox. We associate this reduction in occurrence rate, however, to a non-geophysical factor. An increase in the daytime sky noise in the months around March Equinox causes a decrease in the signal-to-noise ratio (SNR) of the echoes, which makes them less distinguishable in our analysis. A higher occurrence of weaker echoes around March Equinox was confirmed by an statistical analysis of the seasonal variation of echo intensities. Strong, long-lasting and, therefore, more noticeable echoing layers, however, were observed between June and early September compared to other months in 2008. Spectral analyses show that most of the echoes have negative mean Doppler shifts indicating upward velocities. The echoes also have narrow spectral widths of only a few ms−1. Finally, we also found that the mean Doppler shift of the observed echoes can vary noticeably with altitude at times. Using spaced antenna measurements we show that this is caused by the wide field-ofview of the radar and the spatial distribution of the scatterers within the radar beam.es_ES
dc.description.peer-reviewPor pareses_ES
dc.formatapplication/pdfes_ES
dc.identifier.citationRodrigues, F. S., De Paula, E. R., & Chau, J. L. (2011). On the characteristics of 150-km echoes observed in the Brazilian longitude sector by the 30 MHz São Luís radar.==$Annales Geophysicae, 29$==(10), 1905–1916. https://doi.org/10.5194/angeo-29-1905-2011es_ES
dc.identifier.doihttps://doi.org/10.5194/angeo-29-1905-2011es_ES
dc.identifier.govdocindex-oti2018
dc.identifier.journalAnnales Geophysicaees_ES
dc.identifier.urihttp://hdl.handle.net/20.500.12816/1999
dc.language.isoenges_ES
dc.publisherEuropean Geosciences Union (EGU)es_ES
dc.relation.ispartofurn:issn:0992-7689
dc.rightsinfo:eu-repo/semantics/restrictedAccesses_ES
dc.subjectIonospherees_ES
dc.subjectEquatorial ionospherees_ES
dc.subjectRadares_ES
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.05.01es_ES
dc.titleOn the characteristics of 150-km echoes observed in the Brazilian longitude sector by the 30 MHz São Luís radares_ES
dc.typeinfo:eu-repo/semantics/articlees_ES

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